Abstract
The cross-correlation between time series of solar cycle length and amplitude suggests that the length precedes the amplitude. The relationship between the two is found to be more complex than a simple lag er phase shift, however. A simple empirical model is constructed which allows the amplitude of a given cycle to be predicted with relatively high accuracy from the lengths of earlier cycles. This result not only adds to the means at our disposal for predicting the amplitudes of future cycles, but also implies that the solar dynamo carries a memory of the length of one cycle over into the next. It may also have a bearing on why solar cycle length correlates better with the Earth's temperature record than cycle amplitude (Friis-Christensen & Lassen 1991). Thoughts on possible physical causes are presented.
| Original language | English |
|---|---|
| Pages (from-to) | 1029-1035 |
| Number of pages | 7 |
| Journal | Astronomy and Astrophysics |
| Volume | 396 |
| Issue number | 3 |
| DOIs | |
| Publication status | Published - Dec 2002 |
Keywords
- Solar-terrestrial relations
- Sun: magnetic fields
- Sunspots
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